M-dwarf Eclipsing Binaries with Flare Activity

doi:10.3847/1538-4357/ab774a

YNAO OpenIR > 南方基地

	M-dwarf Eclipsing Binaries with Flare Activity
	Huang, L. -C.1; Ip, W. -H.1,2,3; Lin, C. -L.1; Zhang XL(张西亮)4 ; Song, Y. -H.5; Luo, A. -L.5
发表期刊	ASTROPHYSICAL JOURNAL
	2020-03-20
卷号	892 期号:1 页码:11
DOI	10.3847/1538-4357/ab774a
产权排序	第4完成单位
收录类别	SCI
关键词	Stellar flares
摘要	The physical properties of 12 eclipsing binaries of M-type dwarfs with superflare activity are characterized by combining the ground-based spectroscopic measurements and the photometric light curves obtained by the Kepler Space Telescope. All of these binary systems have Algol-type orbital configurations. The primary components are mostly of the early M-type dwarfs (M0-M3). Even though the occurrence rate of large flares with energy >10(34) erg of the EBs is less than the hyperflaring M dwarfs, the corresponding cumulative flare frequency is in general about a factor of 10 higher than the single M dwarfs with flare activity. This might be the consequence of magnetic interaction between the primary and secondary component of individual binaries. The slow rotators are not as active as the fast rotators, some of which display a possible eclipsing effect in their flare activity.
资助项目	MOST, Taiwan[107-2119-M-008-012] ; FCDT of Macau, MSAR[119/2017/A3] ; Chinese Academy of Sciences ; Peoples Government of Yunnan Province ; National Development and Reform Commission
项目资助者	MOST, Taiwan[107-2119-M-008-012] ; FCDT of Macau, MSAR[119/2017/A3] ; Chinese Academy of Sciences ; Peoples Government of Yunnan Province ; National Development and Reform Commission
语种	英语
学科领域	天文学 ; 恒星与银河系
文章类型	Article
出版者	IOP PUBLISHING LTD
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN	0004-637X
URL	查看原文
WOS记录号	WOS:000522410600001
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	COOL CLOSE BINARIES ; LOW-MASS STAR ; STELLAR FLARE ; X-RAY ; ROTATION ; SUPERFLARES ; EVOLUTION ; FIELD ; TEMPERATURES ; MISSION
引用统计	被引频次：11[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/23015
专题	南方基地
通讯作者	Huang, L. -C.
作者单位	1.Institute of Astronomy, National Central University, Taiwan 2.Institute of Space Science, National Central University, Taiwan 3.Space Science Institute, Macau University of Science and Technology, Macau MSAR 4.Yunnan Observatories, Chinese Academy of Science, People's Republic of China 5.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, People's Republic of China
推荐引用方式 GB/T 7714	Huang, L. -C.,Ip, W. -H.,Lin, C. -L.,et al. M-dwarf Eclipsing Binaries with Flare Activity[J]. ASTROPHYSICAL JOURNAL,2020,892(1):11.
APA	Huang, L. -C.,Ip, W. -H.,Lin, C. -L.,Zhang XL,Song, Y. -H.,&Luo, A. -L..(2020).M-dwarf Eclipsing Binaries with Flare Activity.ASTROPHYSICAL JOURNAL,892(1),11.
MLA	Huang, L. -C.,et al."M-dwarf Eclipsing Binaries with Flare Activity".ASTROPHYSICAL JOURNAL 892.1(2020):11.

条目包含的文件
文件名称/大小	文献类型	版本类型	开放类型	使用许可
M-dwarf Eclipsing Bi（2643KB）	期刊论文	出版稿	开放获取	CC BY-NC-SA	浏览请求全文